Chemodynamical evolution of the Milky Way

C. Kobayashi, N. Nakasato, K. Nomoto

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We simulate the chemodynamical evolution of the Milky Way using our GRAPE-SPH code, and reproduce the age-metallicity relation, the [O/Fe]-[Fe/H] relation, and the metallicity distribution.

Original languageEnglish
Title of host publicationAstrophysical Supercomputing Using Particle Simulations
EditorsJ. Makino, P. Hut
Place of PublicationSAN FRANCISCO
PublisherAstronomical Society of the Pacific
Pages419-420
Number of pages2
ISBN (Print)1-58381-139-7
Publication statusPublished - 2003
Event208th Symposium of the International Astronomical Union - Tokyo, Japan
Duration: 10 Jul 200113 Jul 2001

Conference

Conference208th Symposium of the International Astronomical Union
Country/TerritoryJapan
CityTokyo
Period10/07/0113/07/01

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